Lecture

Electron Holography: Theory & Practical Examples

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In course

MSE-670: Advanced Microscopy for Magnetic Materials

Theoretical and practical expertise is gained about the microscopy of spin structures and magnetic configuiations down to the sub-nm length and sub-ns time scales such as transmission electron microscopy, x-ray and light scattering, magnetic dichroism, and ...

Description

This lecture covers the theory and practical examples of off-axis electron holography, focusing on magnetic fields and other forms of electron holography. It explains the basis of electron holography, historical background, digital reconstruction, and the application of vertical magnetic fields. The lecture also discusses the off-axis electron holography of magnetic materials, including the separation of magnetic and electrostatic contributions, in situ magnetization reversal, and the determination of coercivity. Furthermore, it explores low-temperature studies of skyrmions, magnetic high-entropy alloys, and 3D magnetic vector field holographic tomography. The presentation concludes with discussions on electron-beam-induced charging, electron holography at elevated temperatures, and the measurement of magnetic moments through model-independent approaches.

Instructors (4)

Thomas La Grange

Expertise Electron Microscopy, Aberration Correct Scanning Transmission Electron Microscopy, Electron Diffraction, Ultrafast Transmission Electron Microscopy, Electron Energy Loss Spectroscopy, Energy Dispersive Spectroscopy, Materials Science, High-speed deformation, Dislocation Dynamics, Skyrmionics, Martensitic Phase Transformation Theory, Solidification Expertise Electron Microscopy, Aberration Correct Scanning Transmission Electron Microscopy, Electron Diffraction, Ultrafast Transmission Electron Micro

Fabrizio Carbone

Birth 20/04/1976 Master degree: University of Pavia "optoelectronic engineering". September 2001. Reasearch scientist at Pirelli Labs, Milan Italy between September 2000 and August 2002. PhD in condensed matter physics from the University of Geneva, prof. van der Marel gorup. January 2007 Post doc in physical chemistry at Caltech in prof. Zewail`s group. March 2007-April 2009

Dirk Grundler

Phoebe Marie Tengdin

Official source

Related concepts (32)

Magnetic field

A magnetic field is a vector field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular to its own velocity and to the magnetic field. A permanent magnet's magnetic field pulls on ferromagnetic materials such as iron, and attracts or repels other magnets.

Earth's magnetic field

Earth's magnetic field, also known as the geomagnetic field, is the magnetic field that extends from Earth's interior out into space, where it interacts with the solar wind, a stream of charged particles emanating from the Sun. The magnetic field is generated by electric currents due to the motion of convection currents of a mixture of molten iron and nickel in Earth's outer core: these convection currents are caused by heat escaping from the core, a natural process called a geodynamo.

Electromagnetic field

An electromagnetic field (also EM field or EMF) is a classical (i.e. non-quantum) field produced by moving electric charges. It is the field described by classical electrodynamics (a classical field theory) and is the classical counterpart to the quantized electromagnetic field tensor in quantum electrodynamics (a quantum field theory). The electromagnetic field propagates at the speed of light (in fact, this field can be identified as light) and interacts with charges and currents.

Interplanetary magnetic field

The interplanetary magnetic field (IMF), now more commonly referred to as the heliospheric magnetic field (HMF), is the component of the solar magnetic field that is dragged out from the solar corona by the solar wind flow to fill the Solar System. The coronal and solar wind plasmas are highly electrically conductive, meaning the magnetic field lines and the plasma flows are effectively "frozen" together and the magnetic field cannot diffuse through the plasma on time scales of interest.

Magnetic moment

In electromagnetism, the magnetic moment is the magnetic strength and orientation of a magnet or other object that produces a magnetic field. Examples of objects that have magnetic moments include loops of electric current (such as electromagnets), permanent magnets, elementary particles (such as electrons), composite particles (such as protons and neutrons), various molecules, and many astronomical objects (such as many planets, some moons, stars, etc).

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